Physics — HSSC-II Practice Quiz

50 MCQs built on the FBISE Physics Grade-XII Model Paper & Table of Specifications + Federal Board Textbook (Units 15–25). Then short questions and the most important long questions, chapter by chapter.

Curriculum 2022-23 Grade XII Mobile-friendly Auto-scored

Section B style — 3 marks each. Answer in a short definition / 2–3 brief points or a small derivation. Distribution follows the model paper weighting (Modern Physics & Electricity carry the most marks).

Unit 15 — Gravitation
1. Define gravitational field strength. Also write its formula and unit.

Gravitational field strength g at a point is the gravitational force experienced per unit mass placed at that point. Formula: g = GM/r² (= F/m). SI unit: N kg⁻¹ (or m s⁻²). It is a vector directed toward the mass producing the field.

2. Why is g approximately constant for small changes in height near the Earth's surface?

Since g = GM/r², g depends on r (distance from Earth's centre ≈ 6.4×10⁶ m). For small heights h ≪ R, the change r = R + h is negligible compared with R, so g changes by an insignificant amount and may be treated as constant near the surface.

3. What is a geostationary satellite?

A satellite whose orbital period equals the Earth's rotational period (≈ 24 hours), orbiting from west to east directly above the Equator. It therefore stays fixed above the same point on Earth — used for communication and weather monitoring. Its orbital radius is about 4.23×10⁷ m.

Unit 16 — Statistical Mechanics & Thermodynamics
4. Explain how pressure is exerted by the movement of gas molecules.

Gas molecules move randomly and continuously collide with the walls of the container. At each collision a molecule's momentum changes, exerting a force on the wall. The total force per unit area from these countless collisions is the pressure of the gas.

5. How is pressure related to the average translational kinetic energy of a gas?

From kinetic theory, pV = ⅓Nm⟨c²⟩ and average translational KE = ½m⟨c²⟩. Combining gives pV = ⅔N(½m⟨c²⟩), i.e. pressure is directly proportional to the average translational kinetic energy (and hence to absolute temperature) of the molecules.

6. Why do real gases deviate from ideal gas behaviour?

Because real gas molecules (i) have intermolecular forces of attraction and (ii) occupy a finite volume — both ignored in the ideal model. Deviations become large at high pressure and low temperature, where molecules are close together.

Unit 17 — Simple Harmonic Motion
7. Define SHM and state its essential condition.

Simple harmonic motion is a to-and-fro motion in which the acceleration is directly proportional to the displacement from a fixed (mean) point and is always directed towards that point: a = −ω²x. The restoring force is proportional to displacement (F = −kx).

8. Describe the interchange between kinetic and potential energy during SHM.

Total energy ½mω²x₀² stays constant. At the mean position KE is maximum and PE is zero; at the extreme positions PE is maximum and KE is zero. Energy continuously converts KE ⇌ PE while the sum remains fixed.

9. Write three real-life examples of resonance.

(i) Tuning a radio/TV to a station (electrical resonance). (ii) Heating food in a microwave oven. (iii) Pushing a swing at its natural frequency. (Also: shattering a glass by sound, vibration of a bridge.)

10. Describe practical examples of free and forced oscillations.

Free oscillation: a system displaced and released vibrates at its own natural frequency, e.g. a struck tuning fork or a simple pendulum. Forced oscillation: a system driven by an external periodic force, e.g. a vibrating bridge under marching feet or a loudspeaker cone driven by AC.

Unit 18 — Diffraction & Interference
11. Write any three conditions for observing interference fringes.

(i) The two sources must be coherent (constant phase difference). (ii) They must have the same frequency/wavelength and nearly equal amplitude. (iii) The sources must be close together and the screen far away (and waves of the same polarization).

12. What is a diffraction grating?

An optical device consisting of a very large number of equally spaced, close parallel slits (lines) per unit length. It diffracts light into sharp, widely separated maxima and is used to determine the wavelength of light using d sin θ = nλ.

13. State the conditions for constructive and destructive interference (path difference).

Constructive: path difference = nλ (n = 0,1,2,…) — waves in phase, bright fringe. Destructive: path difference = (n + ½)λ — waves out of phase, dark fringe.

Unit 19 — Electric Potential & Capacitor
14. Define electric potential and write its formula for a point charge.

Electric potential at a point is the work done per unit positive charge in bringing a small test charge from infinity to that point. For a point charge: V = q / (4πε₀r). SI unit: volt (J C⁻¹).

15. List the use of capacitors in various household appliances.

Used in flash guns of cameras, electric fans (starting capacitor), refrigerators, and in rectification/smoothing circuits of power supplies — to store charge and release it quickly or to smooth current.

16. Derive the combined capacitance of two capacitors in series.

In series the charge Q on each is the same; voltages add: V = V₁ + V₂ = Q/C₁ + Q/C₂. Since V = Q/C, dividing by Q gives 1/C = 1/C₁ + 1/C₂. The combined capacitance is smaller than the smallest individual capacitor.

Unit 20 — Alternating Current
17. Define mutual inductance and self-inductance. Also write their unit.

Self-inductance (L): the property of a coil that opposes any change of current in itself by inducing a back-emf. Mutual inductance (M): the emf induced in one coil due to a changing current in a neighbouring coil. SI unit of both: henry (H).

18. Distinguish between root-mean-square (rms) and peak values of an AC.

The peak value (I₀, V₀) is the maximum instantaneous value of the alternating quantity. The rms value is the steady DC value that produces the same heating effect: I = I₀/√2 and V = V₀/√2 for a sinusoidal AC.

19. Explain the role of a single capacitor in the output of a full-wave rectifier.

The capacitor is connected across the load. It charges at the peaks and discharges slowly through the load between peaks, filling in the dips. This smooths the pulsating rectified output toward steady DC; larger C and load resistance give less ripple.

20. Calculate the capacitive reactance for: V = 16 sin(2×10³ t) across a 0.5 μF capacitor.

Here ω = 2×10³ rad s⁻¹ and C = 0.5×10⁻⁶ F. Capacitive reactance X_C = 1/(ωC) = 1 / (2×10³ × 0.5×10⁻⁶) = 1 / (10⁻³) = 1000 Ω (1 kΩ).

Unit 21 — Quantum Physics
21. Describe how photoelectrons are emitted from a metal surface.

When electromagnetic radiation of frequency ≥ the threshold frequency strikes a metal, each photon (energy hf) gives its energy to one electron. If hf exceeds the work function ϕ, the electron escapes as a photoelectron with KE = hf − ϕ.

22. State Heisenberg's uncertainty principle.

It is impossible to measure both the position and momentum of a particle simultaneously with perfect accuracy. The product of the uncertainties is at least of the order of h: Δx · Δp ≥ h/4π. (If Δx → 0, then Δp → ∞.)

23. Explain how electron microscopes achieve very high resolution.

Resolution is limited by wavelength. Fast electrons have a very small de Broglie wavelength (λ = h/p) — far shorter than visible light — so an electron microscope can resolve much finer detail than an optical microscope.

24. Explain that a photon has momentum. Calculate the energy of a gamma photon of wavelength 1 Å.

A photon has zero rest mass but carries momentum p = E/c = h/λ, so light can exert a force (radiation pressure). For λ = 1 Å = 10⁻¹⁰ m: E = hc/λ = (6.63×10⁻³⁴ × 3×10⁸)/10⁻¹⁰ ≈ 1.99×10⁻¹⁵ J = ≈ 12.4×10³ eV.

Unit 22 — Nuclear Physics
25. Sketch / describe the variation of binding energy per nucleon with nucleon number.

Binding energy per nucleon rises steeply for light nuclei, peaks at ≈ 8.8 MeV around iron (A ≈ 56), then falls slowly for heavy nuclei. The peak means iron-group nuclei are most stable; fusion of light nuclei and fission of heavy nuclei both move toward this peak, releasing energy.

26. Define mass defect and binding energy.

Mass defect: the difference between the total mass of the separate nucleons and the actual (smaller) mass of the nucleus. Binding energy: the energy equivalent of this mass defect (E = Δmc²) — the energy needed to break the nucleus into its nucleons.

27. Describe the function of control rods in a nuclear reactor.

Control rods (e.g. boron or cadmium) absorb excess neutrons. By inserting or withdrawing them, the rate of the fission chain reaction is controlled — pushed in to slow it down or pulled out to speed it up, keeping the reaction steady and safe.

28. Explain half-life with an example.

The half-life (T½) is the time in which half the radioactive nuclei in a sample decay. It is constant for a given isotope. e.g. for an isotope of T½ = 8 days, 16 g decays to 8 g after 8 days, 4 g after 16 days, and so on. Related to decay constant by λ = 0.693/T½.

Unit 23 — Cosmology
29. Define and explain the term luminosity.

Luminosity is the total power of radiation emitted by a star in all directions (energy radiated per second). SI unit: watt (W). It depends on the star's surface area and temperature (L = 4πr²σT⁴).

30. Define and explain annihilation reaction.

Annihilation occurs when a particle meets its antiparticle (e.g. electron + positron). Their entire mass converts into energy, producing a pair of gamma-ray photons moving in opposite directions, conserving mass-energy and momentum.

31. What is Stefan–Boltzmann law? Explain briefly.

It states that the total power radiated per unit surface area of a black body is proportional to the fourth power of its absolute temperature. For a star: L = 4πr²σT⁴, where σ is the Stefan–Boltzmann constant. A small rise in T greatly increases luminosity.

Unit 24 — Earth's Climate
32. Define (a) cryosphere (b) lithosphere.

(a) Cryosphere: the part of Earth's climate system made of frozen water — ice sheets, glaciers, sea ice and permafrost. (b) Lithosphere: Earth's solid upper rocky layer (the surface land/crust) that interacts with the atmosphere and oceans.

33. What is climate inertia?

Climate inertia is the phenomenon by which climate systems show resistance or slowness to change when a significant factor is altered. e.g. even if greenhouse emissions stabilise, the climate responds slowly because of complex feedback systems (oceans store heat for a long time).

34. Explain briefly how global climate is determined by energy transfer from the Sun.

Earth's climate is driven by the Earth energy budget — the balance between incoming solar radiation and outgoing radiation. Unequal heating between the equator and poles creates an energy imbalance that drives atmospheric circulation and ocean currents, shaping global climate.

Unit 25 — Medical Imaging
35. What is the application of the piezo-electric effect in medical science?

A piezoelectric transducer uses the piezoelectric effect to both generate and detect ultrasound waves: an AC voltage makes the crystal vibrate (producing ultrasound), and returning echoes deform the crystal to produce a voltage — used for diagnostic ultrasound imaging.

36. What is the main purpose of X-rays in medical imaging?

X-rays pass through soft tissue but are absorbed by denser structures (bones, teeth), producing a contrast image of internal structures. They are used to detect fractures, tumours and other abnormalities inside the body.

37. What are the conditions required for pair production to occur?

A high-energy gamma photon (energy ≥ 1.02 MeV, i.e. ≥ 2m₀c²) must interact near a heavy nucleus (to conserve momentum). The photon then converts into an electron–positron pair, conserving charge, energy and momentum.

★ Most Important Short Questions (high-frequency)
M1. Define gravitational field strength; give its formula and unit. (Sec B)

Force per unit mass at a point; g = GM/r²; unit N kg⁻¹. Directed toward the mass.

M2. Distinguish between rms and peak values for a sinusoidal AC. (Sec B)

Peak = maximum instantaneous value; rms = I₀/√2 (same heating effect as equivalent DC).

M3. State Heisenberg's uncertainty principle. (Sec B)

Δx·Δp ≥ h/4π — position and momentum cannot both be known exactly.

M4. Define mass defect and binding energy. (Sec B)

Mass defect = (sum of nucleon masses − nuclear mass); binding energy = Δmc².

M5. What is the application of the piezoelectric effect in medical science? (Sec B)

A piezoelectric transducer generates and detects ultrasound for diagnostic imaging.

M6. Write three examples of resonance from everyday life. (Sec B)

Tuning a radio, microwave oven, pushing a swing at its natural frequency.

Section C (Extended Response) style — usually split (e.g. 1+6, 4+2, 3+3). The orange "MOST IMPORTANT" tag marks the most likely long question per chapter, based on the model paper (Q3–Q6) and SLO weighting.

Unit 15 — Gravitation
LONG Q · 1 + 6 MARKSMOST IMPORTANT

Define the term gravitational potential. Derive the expression for gravitational potential in the field due to a point mass.

This is model paper Q3. Define potential as work done per unit mass in bringing a small test mass from infinity to the point; derive φ = −GM/r by integrating the work done against the gravitational force; explain the negative sign and link to gravitational potential energy E_p = −GMm/r.

LONG Q · 7 MARKS

State Newton's law of gravitation and analyse circular orbits and geostationary satellites.

F = Gm₁m₂/r²; equate gravitational force to centripetal force (mv²/r) to derive orbital speed v = √(GM/r) and period; explain the conditions for a geostationary satellite (period 24 h, above the Equator, west→east).

Unit 16 — Statistical Mechanics & Thermodynamics
LONG Q · 7 MARKSMOST IMPORTANT

Derive the kinetic theory relation pV = ⅓Nm⟨c²⟩ and use it to find the average translational kinetic energy of a gas.

Consider molecules colliding with the walls of a cube; find momentum change and force in one dimension, extend to three dimensions using ⟨c²⟩ = 3⟨c_x²⟩; obtain pV = ⅓Nm⟨c²⟩ and hence average KE = (3/2)kT and the rms speed.

Unit 17 — Simple Harmonic Motion
LONG Q · 5 + 2 MARKSMOST IMPORTANT

Analyse the interchange between kinetic and potential energy during simple harmonic motion.

This is model paper Q3 (OR). Show total energy = ½mω²x₀² is constant; derive KE = ½mω²(x₀²−x²) and PE = ½mω²x²; describe the energy exchange at mean and extreme positions; sketch energy vs displacement graphs.

LONG Q · 7 MARKS

Explain SHM, derive a = −ω²x, and discuss damped oscillations (light, critical and heavy damping).

Condition for SHM; expressions x = x₀cos(ωt) and v = ±ω√(x₀²−x²); resistive force causing damping; displacement–time graphs for light, critical and heavy damping; importance of critical damping in a car suspension.

Unit 18 — Diffraction & Interference
LONG Q · 1 + 3 + 2 MARKSMOST IMPORTANT

Define interference, discuss the conditions for observing interference, and give the path difference for constructive and destructive interference.

This is model paper Q4. Define interference; state coherence/same wavelength/close sources conditions; constructive: path difference = nλ; destructive: (n+½)λ; relate to Young's double-slit fringe spacing Δy = λL/d.

LONG Q · 6 MARKS

Describe Young's double-slit experiment and derive the fringe-spacing formula Δy = λL/d.

Set-up with coherent sources; geometry of path difference d sinθ = nλ; small-angle approximation; derive fringe spacing and use it in numerical problems (e.g. finding slit separation or wavelength).

Unit 19 — Electric Potential & Capacitor
LONG Q · 4 + 2 MARKSMOST IMPORTANT

Explain the process of charging of a capacitor through a resistor, and discuss the term time constant.

This is model paper Q4 (OR). Describe the exponential growth of charge/voltage and decay of current; equations of the form x = x₀ e^(−t/RC); define and interpret the time constant τ = RC; sketch the charge–time and current–time graphs.

LONG Q · 7 MARKS

Derive expressions for capacitors combined in series and in parallel, and for the energy stored in a capacitor.

Series: 1/C = 1/C₁ + 1/C₂ + …; parallel: C = C₁ + C₂ + …; energy stored E = ½QV = ½CV² from the area under the charge–voltage graph; include a network numerical.

Unit 20 — Alternating Current
LONG Q · 1 + 6 MARKSMOST IMPORTANT

What is rectification? Explain the operation of a bridge (full-wave) rectifier with the help of a diagram.

This is model paper Q5. Define rectification; draw the four-diode bridge; explain which two diodes conduct in each half cycle so current flows the same way through the load both halves; show input/output waveforms and the role of a smoothing capacitor.

LONG Q · 6 MARKS

Explain reactance and impedance in AC circuits; distinguish half-wave from full-wave rectification.

Capacitive reactance X_C = 1/ωC, inductive reactance X_L = ωL; impedance as the vector sum of resistance and reactance; chokes; graphical comparison of half-wave (one diode) and full-wave rectification.

Unit 21 — Quantum Physics
LONG Q · 1 + 6 MARKSMOST IMPORTANT

What is the photoelectric effect? Explain it in detail.

This is model paper Q5 (OR). Define photoelectric effect; describe emission of photoelectrons; threshold frequency and work function; Einstein's equation hf = ϕ + ½mv²_max; explain why max KE is independent of intensity while photocurrent is proportional to intensity.

LONG Q · 7 MARKS

Discuss the wave–particle duality of light and matter (de Broglie wavelength and electron diffraction).

Photoelectric effect and Compton effect as evidence for particle nature; interference/diffraction as evidence for wave nature; de Broglie relation λ = h/p; electron diffraction as evidence for the wave nature of particles.

Unit 22 — Nuclear Physics
LONG Q · 6 MARKSMOST IMPORTANT

Explain half-life with examples; use λ = 0.693/T to solve a numerical problem.

This is model paper Q6 (OR). Define half-life and decay constant; exponential decay law N = N₀ e^(−λt); relation λ = 0.693/T; worked example finding remaining nuclei/activity after a number of half-lives.

LONG Q · 7 MARKS

Explain nuclear fission and fusion, the binding-energy-per-nucleon curve, and the working of a water-moderated reactor.

Mass defect and binding energy; the BE/nucleon curve and why fusion and fission release energy; chain reaction; functions of core, fuel, moderator, control rods, coolant, heat exchanger and shielding.

Unit 23 — Cosmology
LONG Q · 3 + 3 MARKSMOST IMPORTANT

Define and explain the following terms: (a) luminosity (b) annihilation reaction.

This is model paper Q6. (a) Luminosity — total radiant power of a star (W); inverse square law F = L/4πd²; Stefan–Boltzmann L = 4πr²σT⁴. (b) Annihilation — particle meets antiparticle, mass converts to a pair of gamma photons; conservation of energy and momentum; link to PET scanning.

LONG Q · 6 MARKS

Explain redshift and how it leads to the idea of an expanding Universe.

Emission/absorption lines shifted to longer wavelengths; Δλ/λ ≈ Δf/f ≈ v/c; Hubble's observation that distant galaxies recede; redshift as evidence for the expanding Universe and the Big Bang.

Unit 24 — Earth's Climate
LONG Q · 7 MARKSMOST IMPORTANT

Describe Earth's climate system as a complex system of five interacting components, and explain how global climate is determined by energy transfer from the Sun.

The five components: atmosphere, hydrosphere, cryosphere, lithosphere and biosphere; the Earth energy budget; energy imbalance between poles and equator driving atmospheric circulation; climate inertia and feedback.

Unit 25 — Medical Imaging
LONG Q · 7 MARKSMOST IMPORTANT

Explain the production and medical use of X-rays, and how ultrasound and PET scanning are used in diagnosis.

X-rays produced by electron bombardment of a metal target; minimum wavelength from accelerating p.d.; contrast in X-ray imaging; piezoelectric transducer for ultrasound; PET — annihilation gamma photons detected to image tracer concentration.

Tip: In the real paper — Section A = 17 MCQs (compulsory, 17 marks). Section B = 14 short questions of 3 marks each (Q2 i–xiv, each with an OR choice = 42 marks). Section C = Q3–Q6 extended-response questions with OR choices (26 marks). Modern Physics + Electricity & Magnetism together carry the largest share, so prioritise them — but practise the OR alternatives too.